- Page 4 and 5: Contents Foreword Preface xv xvii 1
- Page 6 and 7: v 9 Spin Effects 151 9.1 Diurnal Ev
- Page 8 and 9: List of Figures 1.1 Four comet nucl
- Page 10 and 11: ix 6.4 Schematic representation of
- Page 12 and 13: xi 10.4 Flux rates of H 2 O, CO 2 ,
- Page 14 and 15: List of Tables 1 List of Symbols (s
- Page 16 and 17: Foreword Modern comet research focu
- Page 18 and 19: Preface The discussions in this boo
- Page 20 and 21: xix We consider several different n
- Page 22 and 23: xxi Table 1: List of Symbols (see a
- Page 24 and 25: xxiii Symbol Meaning Units (SI) α
- Page 26 and 27: xxv Table 2: List of Constants Cons
- Page 28 and 29: — 1 — Introduction - Observatio
- Page 30 and 31: 3 TA004947 Figure 1.1: Four comet n
- Page 32 and 33: 5 cloud into the inner Solar System
- Page 34 and 35: 7 Therefore, the abundance of volat
- Page 36 and 37: — 2 — The Structure of Comet Nu
- Page 38 and 39: 2.1. Size and Composition 11 Table
- Page 40 and 41: 2.1. Size and Composition 13 Table
- Page 42 and 43: 2.2. Some Physical Properties 15 (P
- Page 44 and 45: 2.2. Some Physical Properties 17 Ta
- Page 46 and 47: 2.3. Comet - Asteroid Transitions 1
- Page 48 and 49: 2.4. Laboratory Simulations 21 2.4
- Page 50 and 51: 2.4. Laboratory Simulations 23 2.4.
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2.4. Laboratory Simulations 25 wate
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2.4. Laboratory Simulations 27 at o
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2.4. Laboratory Simulations 29 ice,
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— 3 — Physical Processes in Com
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3.2. The Phase Transition of Amorph
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3.3. Gas Diffusion in Pores 35 3.3
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3.3. Gas Diffusion in Pores 37 C BA
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3.3. Gas Diffusion in Pores 39 whic
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3.4. The Coma/Nucleus Boundary Laye
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3.4. The Coma/Nucleus Boundary Laye
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3.4. The Coma/Nucleus Boundary Laye
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3.4. The Coma/Nucleus Boundary Laye
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3.5. Dust Entrainment and Dust Mant
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3.5. Dust Entrainment and Dust Mant
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3.6. Fracturing, Splitting, and Out
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3.6. Fracturing, Splitting, and Out
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— 4 — Basic Equations “As we
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4.2. Energy Balance 59 Summation of
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4.3. Momentum Balance 61 We note th
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4.5. Initial Structure and Paramete
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4.5. Initial Structure and Paramete
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4.6. Flow Regimes and their Transit
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4.7. Dust Flow and Mantling 69 of g
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4.7. Dust Flow and Mantling 71 The
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4.9. Effective Thermal Conductivity
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4.9. Effective Thermal Conductivity
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4.9. Effective Thermal Conductivity
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— 5 — Analytical Considerations
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5.1. Early Models 81 2850 Enthalpy
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5.1. Early Models 83 Net Flux and S
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5.2. Characteristic Properties of t
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5.3. Characteristic Timescales 87 c
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5.3. Characteristic Timescales 89 f
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5.4. An Analytical Model for Crysta
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5.4. An Analytical Model for Crysta
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5.4. An Analytical Model for Crysta
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5.4. An Analytical Model for Crysta
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— 6 — Numerical Methods “. .
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6.1. 1-D Difference Schemes 101 We
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6.2. Treatment of Boundary Conditio
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6.2. Treatment of Boundary Conditio
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6.3. From 1-D to Multi-Dimensions 1
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6.4. Simultaneous Solution for Tran
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6.5. Stability Problems 111 where a
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6.5. Stability Problems 113 As the
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— 7 — Comparison of Algorithms
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Table 7.1: Numerical treatment of p
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7.2. Thermal Algorithm: Different F
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7.4. Results of Different Algorithm
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7.4. Results of Different Algorithm
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7.4. Results of Different Algorithm
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7.4. Results of Different Algorithm
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7.4. Results of Different Algorithm
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7.5. Conclusions 131 sublimated gas
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7.5. Conclusions 133 In Model 3a, c
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— 8 — Orbital Effects “Halley
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8.2. Short-Period vs. Long-Period C
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8.2. Short-Period vs. Long-Period C
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8.2. Short-Period vs. Long-Period C
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8.2. Short-Period vs. Long-Period C
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8.3. Changing Orbits 145 Jupiter is
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8.5. Sungrazing Comets 147 stage IV
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8.5. Sungrazing Comets 149 More rec
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— 9 — Spin Effects “The motio
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9.3. Day - Night Temperature Differ
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9.4. Effect of Spin Axis Inclinatio
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9.4. Effect of Spin Axis Inclinatio
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9.4. Effect of Spin Axis Inclinatio
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9.5. Effect of Spin Rate 161 Spin a
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9.5. Effect of Spin Rate 163 Figure
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— 10 — Comparison of Models wit
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10.1. Modeling Guided by Observatio
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10.1. Modeling Guided by Observatio
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10.1. Modeling Guided by Observatio
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10.1. Modeling Guided by Observatio
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10.1. Modeling Guided by Observatio
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10.1. Modeling Guided by Observatio
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10.1. Modeling Guided by Observatio
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10.2. Conclusions Based on Multiple
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10.2. Conclusions Based on Multiple
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10.3. Comet Outbursts 185 et al., 1
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10.3. Comet Outbursts 187 Marcialis
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10.4. Coma Versus Nucleus Abundance
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10.4. Coma Versus Nucleus Abundance
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10.4. Coma Versus Nucleus Abundance
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10.4. Coma Versus Nucleus Abundance
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— 11 — Internal Properties of C
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11.2. Stratification of Composition
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11.3. Dust Mantle Thickness 201 Bec
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11.3. Dust Mantle Thickness 203 whe
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— 12 — Conclusions “. . . Mor
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12.2. Goals of Comet Nucleus Modeli
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12.4. General Behaviour Patterns 20
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12.5. Input Data Required from Obse
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12.5. Input Data Required from Obse
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Appendix A: Orbital Parameters and
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Comet q (AU) e R (a) (km) R (b) (km
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Comet q (AU) e R (a) (km) R (b) (km
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Appendix B: Thermodynamic Propertie
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B.2. Specific Heat 223 Since water
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Glossary Scientific terms used in r
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Bibliography This list collects pap
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229 R., Paubert, G., Evolution of t
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231 Observatory Faint Comet Survey
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233 Eberhardt, P., Krankowsky, D.,
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235 dust, in Comets, (ed. L. L. Wil
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237 Huebner, W. F., Boice, D. C., P
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239 of porous media, Phys. Rev. E 5
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241 U. Keller, H. A. Weaver), Unive
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243 1993. [2.4] Mekler Y., Podolak,
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245 effect of the dust mantle, Icar
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247 Sagdeev, R. Z., Elyasberg, P. E
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249 827, 1997. [2.2] Skorov, Y. V.,
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251 86, 236, 1990. [4.5] Taban, I.
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Subject Index Abundance ratio, 11,
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SUBJECT INDEX 255 Emissivity, 46, 4
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SUBJECT INDEX 257 Planetesimal, 4,